Comparative Analysis of the E.D.E.N. Geodesic Topology

How a dual-icosahedral, hexagon-dominant mesh compares to alternative global discretization methods.

The E.D.E.N. planetary engine is built on a specific geodesic discretization: a dual-icosahedral spherical mesh composed primarily of hexagons with twelve pentagons. This structure provides near-uniform area distribution, consistent adjacency, and a natural basis for environmental modeling.

This document compares that topology to other commonly used planetary discretization methods, including latitude–longitude rasters, cubed-sphere grids, planar projections, unstructured meshes, and more.


1. Overview of the E.D.E.N. Topology

The simulation uses:

  • Base geometry: Icosahedron
  • Subdivision: Recursive refinement of edges, projected to a sphere
  • Cell composition: Hexagon-dominant with exactly 12 pentagons
  • Adjacency: Mostly 6-neighbor tiles, 5-neighbor at pentagons
  • Uniformity: Near-equal-area cells, minimal distortion
  • Data model: Tile, edge, and directed-edge fields

This configuration eliminates poles, preserves surface symmetry, and provides a consistent substrate for scalar, vector, and categorical fields across the entire sphere.


2. Evaluation Criteria

The comparison below evaluates each topology using the following attributes:

  1. Area Uniformity
  2. Adjacency Regularity
  3. Geometric Distortion / Singularities
  4. Hierarchical Refinement
  5. Handling of Flow / Vector Fields
  6. Numerical Stability
  7. Visual and Cognitive Interpretability
  8. Implementation Complexity
  9. Compatibility with Earth-data Standards

3. Latitude–Longitude Grids

Latitude–longitude grids divide the planet using equal angular increments in both directions.

Advantages

  • Very simple indexing
  • Direct compatibility with most global datasets
  • Supported by nearly all GIS and climate tools

Limitations

  • Severe area distortion: cells shrink dramatically near the poles
  • Singularities at the poles disrupt adjacency and flow
  • Strong anisotropy: neighbor distances vary widely with latitude
  • Complications when modeling vector fields and flows

Comparison

The geodesic topology avoids these issues by providing consistent cell areas, no pole singularities, and uniform adjacency globally.


4. Planar Grids + Map Projections

Planar square or hex grids are often mapped to a sphere using a projection.

Advantages

  • Straightforward 2D representation
  • Familiar in game design and visualization contexts

Limitations

  • All projections introduce distortion (area, shape, or distance)
  • Adjacency relationships do not match true spherical geometry
  • Physical processes simulated on the projection require correction

Comparison

The geodesic topology simulates directly on the sphere, eliminating projection distortion during computation.


5. Cubed-Sphere / Quad-Sphere Grids

Cubed-sphere grids start with a cube and project its faces onto the sphere, then subdivide them.

Advantages

  • No true poles
  • More uniform than lat/long
  • Simple (i, j, face) indexing

Limitations

  • Six face seams introduce subtle anisotropies
  • Cell shapes vary from face center to edges
  • Degree-4 adjacency is less isotropic for flow and diffusion modeling

Comparison

While widely used in climate models, cubed-sphere grids remain less isotropic than dual-icosahedral geodesic meshes, which offer smoother symmetry and better support for radial flows.


6. Generic Spherical Meshes (Non-Uniform Hex/Tri)

These meshes often originate from arbitrary triangulations or artist-generated geometry.

Advantages

  • Flexible generation
  • Adaptive meshes are possible

Limitations

  • No inherent guarantees about area or neighbor regularity
  • Harder to analyze or visualize consistently
  • Poor foundation for systematic environmental models

Comparison

The E.D.E.N. topology uses a mathematically controlled mesh with predictable behavior, essential for deterministic simulation.


7. HEALPix (Hierarchical Equal Area Pixelization)

A well-known spherical tessellation used in astrophysics.

Advantages

  • Precisely equal-area cells
  • Strong existing scientific usage

Limitations

  • Not hex-based; cell shapes vary
  • Adjacency patterns differ from uniform hex grids
  • Less natural for edge-based or directional field modeling

Comparison

The E.D.E.N. topology offers more uniform neighbor relationships and aligns more naturally with tile/edge/directed-edge models.


8. Unstructured / Voronoi / FEM-Style Meshes

Common in high-end scientific simulations requiring flexible element shapes.

Advantages

  • Allows adaptive refinement in specific regions
  • Highly accurate for targeted scientific problems

Limitations

  • Complex neighbor relationships
  • Harder to visualize consistently
  • Poor match for general-purpose or educational use
  • Overhead of arbitrary cell geometry

Comparison

While powerful for specialized scientific workloads, unstructured meshes introduce too much complexity for a general, extensible planetary simulation environment.


9. Planar Hex Grids (2D)

Hex grids offer excellent local properties in 2D.

Advantages

  • Uniform area, distance, and adjacency
  • Classic structure for cellular systems

Limitations

  • Not compatible with spherical topology
  • Requires artificial wrap-around (toroidal distortions)

Comparison

The E.D.E.N. mesh extends the advantages of hex grids to a sphere without topological artifacts.


10. Summary of Advantages of the E.D.E.N. Topology

The dual-icosahedral geodesic mesh offers:

  • No poles or singularities
  • Near-equal-area cells globally
  • Consistent 6-neighbor adjacency (except 12 pentagons)
  • Smooth global symmetry
  • Natural subdivision hierarchy
  • Clear tile/edge/directed-edge relationships
  • Strong suitability for vector and flow fields
  • Clean, interpretable visualization

These characteristics make it particularly well-suited for:

  • environmental and climate simulation
  • educational clarity
  • emergent systems modeling
  • scientific visualization
  • robust SDK and extension frameworks

The geodesic topology is therefore an ideal foundation for a modern, extensible planetary simulation ecosystem.